Results 31 to 40 of about 111,155 (292)

New capability for indirect neutron capture measurements: The DICER instrument at LANSCE [PDF]

open access: yesEPJ Web of Conferences, 2022
The Device for Indirect Capture on Radionuclides (DICER) implements a new indirect technique for (n,γ) studies in which the neutron capture rate is determined from analysis of resonance neutron transmission data.
Stamatopoulos A.   +13 more
doaj   +1 more source

Neutron Capture and Neutron Halos

open access: yes, 1996
1)camready.sty file is needed and enclosed 2)To be published in the Proceedings of the 9th International Symposium on Capture Gamma-ray Spectroscopy and Related Topics, Budapest, October 8-12 ...
Mengoni, A.   +3 more
openaire   +2 more sources

Computing Neutron Capture Rates in Neutron-Degenerate Matter

open access: yesUniverse, 2019
Neutron captures are likely to occur in the crust of accreting neutron stars (NSs). Their rate depends on the thermodynamic state of neutrons in the crust. At high densities, neutrons are degenerate.
Bryn Knight, Liliana Caballero
doaj   +1 more source

Evaluation of cadmium ratio for conceptual design of a cyclotron-based thermal neutron radiography system

open access: yesNuclear Engineering and Technology, 2022
An approximate method for calculating the cadmium ratio of a cyclotron-based thermal neutron radiography system was developed. In this method, the Monte-Carlo code, MCNP6.2, was employed to calculate the neutron capture rates of Au-197, and the cadmium ...
Weng-Sheng Kuo
doaj   +1 more source

The capture of neutrons by deuterons [PDF]

open access: yesProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1948
Abstract The cross-sections for capture of neutrons by deuterons, involving emission of both electric and magnetic dipole radiation, are calculated using the wave functions obtained by Buckingham & Massey (1941) in the course of an application of the resonating-group structure method to the elastic scattering of neutrons by ...
Burhop, E. H. S., Massey, H. S. W.
openaire   +1 more source

Capture cross sections on unstable nuclei

open access: yesEPJ Web of Conferences, 2017
Accurate neutron-capture cross sections on unstable nuclei near the line of beta stability are crucial for understanding the s-process nucleosynthesis. However, neutron-capture cross sections for short-lived radionuclides are difficult to measure due to ...
Tonchev A.P.   +20 more
doaj   +1 more source

In vivo evaluation of the effects of combined boron and gadolinium neutron capture therapy in mouse models

open access: yesScientific Reports, 2022
While boron neutron capture therapy (BNCT) depends primarily on the short flight range of the alpha particles emitted by the boron neutron capture reaction, gadolinium neutron capture therapy (GdNCT) mainly relies on gamma rays and Auger electrons ...
Woonghee Lee   +6 more
doaj   +1 more source

Neutron-capture measurement candidates for the r-process in neutron star mergers

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Neutron star mergers (NSMs) are one of the astrophysical sites for the occurrence of the rapid neutron capture process (r-process). After a merger, the ejected neutron-rich matter hosts the production of radioactive heavy nuclei located far from the ...
Diego Vescovi   +4 more
doaj   +1 more source

NEUTRON CAPTURES AND THE R-PROCESS [PDF]

open access: yesThe R-Process, 2004
The r-process involves neutron-rich nuclei far off stability for which no experimental cross sections are known. Therefore, one has to rely on theory. The difficulties in the predictions are briefly addressed. To investigate the impact of altered rates, a comparison of r-process production in hot bubble models with largely varied rates is shown. Due to
openaire   +3 more sources

New Neutron-Capture Site in Massive Pop III and Pop II Stars as a Source for Heavy Elements in the Early Galaxy

open access: yes, 2018
We propose a new neutron-capture site in early metal-poor and metal-free stars of $\sim 20$--$30 \,\mathrm{M}_\odot$ that results from proton ingestion in the He shell during late stages of the stars' lives.
Banerjee, Projjwal   +2 more
core   +1 more source

Home - About - Disclaimer - Privacy